大洋板块在晚阿新世尝试失败后成功俯冲:岩石学和地球化学制约因素

IF 4.8 1区 地球科学 Q1 GEOCHEMISTRY & GEOPHYSICS
Xi Wang , Rong-Feng Ge , Yong-Fei Zheng , Wen-Bin Zhu , San-Zhong Li , Rong-Song Tian , Yue Wang , Yi-Wei Rong
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引用次数: 0

摘要

板块构造始于何时,又是如何演变成我们今天所知的样式的,这是一个基本问题,但也是一个极具争议性的问题。数字地球动力学模型预测,在阿基坦时期向板块构造的过渡是偶发的,可能出现成功和失败的俯冲交替。然而,俯冲失败的直接地质证据却很少。虽然数值模拟已经提出了这种可能性,但仍然缺乏地质证据。在此,我们对华北克拉通(NCC)最西端阿拉善地块的元成岩进行了锆石U-Pb年龄、Hf-O同位素以及全岩主要和微量元素的综合研究。研究发现,在一个3.0Ga前的大陆核周围发生了两个时期的晚阿基坦岩浆活动,分别为2.75Ga和2.5Ga。对约 2.75 Ga 的元岩浆进行了地球化学分析。2.75Ga的元黑质和元长质火成岩显示了两种不同的构造模式。长英岩在成分上类似典型的奥陶纪TTG(tonalite-trondhjemite-granodiorite),εHf(t)值从-2.8到11.0不等,δ18O值从4.3‰到7.9‰不等。岩石成因模型表明,它们的岩浆来源是约3.1-2.75 Ga的大洋。3.1-2.75Ga的大洋地壳在不同温度下发生热液蚀变,然后与较古老的大陆地壳混合,并在石榴石稳定场的下部地壳中部分熔化。这就需要大洋地壳向大陆核的构造增生,这意味着一次尝试或失败的俯冲。相反,元杂岩表现出类似弧的微量元素模式和钙碱性演化趋势,表明大洋板块成功俯冲至亚弧深处,形成了元杂岩幔源。总之,目前的研究结果为大洋板块在阿全新统汇聚边缘的行为提供了强有力的约束,在这里,大洋板块的成功俯冲是在多次尝试失败之后实现的。这种失败-成功的大洋俯冲过程可能适用于整个北西大陆架和世界其他地方的其他陨石坑,反映了板块构造作用在阿歇纪的逐渐成熟,这与数值模拟的预测是一致的。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Successful subduction of oceanic plate after failed attempts in the Late Archean: Petrological and geochemical constraints

When and how plate tectonics started and evolved to the style as we know it today is a fundamental yet highly controversial question. Numerical geodynamic modelling predicts that the transition into plate tectonics in the Archean was episodic with possible alternation between success and failure of subduction. However, direct geological evidence for failed subduction is scarce. While this possibility has been suggested by numerical modelling, it is still lack of geological evidence. Here we present a combined study of zircon U-Pb ages and Hf-O isotopes, as well as whole-rock major and trace elements, for meta-igneous rocks from the Alxa Block in the westmost North China Craton (NCC). Two periods of Late Archean magmatism ca. 2.75 Ga and 2.5 Ga are identified to occur surrounding a pre-3.0 Ga continental nucleus. Geochemical analyses of the ca. 2.75 Ga meta-mafic and meta-felsic igneous rocks show two different modes of tectonic regime. The felsic rocks resemble typical Archean TTG (tonalite-trondhjemite-granodiorite) in composition, with variable εHf(t) values from -2.8 to 11.0 and δ18O values from 4.3 ‰ to 7.9 ‰. Petrogenetic modelling suggests that their magmatic source was the ca. 3.1–2.75 Ga oceanic crust that was hydrothermally altered at different temperatures and then mixed with the older continental crust and partially melted in lower crust in the garnet stability field. This requires tectonic accretion of the oceanic crust to the continental nucleus, signifying an attempted or failed subduction. On the contrary, the meta-mafic rocks exhibit arc-like trace element patterns and calc-alkaline evolution trend, indicating a metasomatic mantle source due to successful subduction of the oceanic slab to subarc depths. Taken together, the present results provide robust constraints on the behavior of oceanic slab at the Archean convergent margin, where successful oceanic subduction would be achieved after several failed attempts. Such failure-success processes of oceanic subduction may be applicable to the whole NCC and other cratons elsewhere in the world, reflecting the gradual maturation of plate tectonics in the Archean, consistent with predictions of numerical modelling.

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来源期刊
Earth and Planetary Science Letters
Earth and Planetary Science Letters 地学-地球化学与地球物理
CiteScore
10.30
自引率
5.70%
发文量
475
审稿时长
2.8 months
期刊介绍: Earth and Planetary Science Letters (EPSL) is a leading journal for researchers across the entire Earth and planetary sciences community. It publishes concise, exciting, high-impact articles ("Letters") of broad interest. Its focus is on physical and chemical processes, the evolution and general properties of the Earth and planets - from their deep interiors to their atmospheres. EPSL also includes a Frontiers section, featuring invited high-profile synthesis articles by leading experts on timely topics to bring cutting-edge research to the wider community.
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